日本地球惑星科学連合2022年大会

講演情報

[E] ポスター発表

セッション記号 S (固体地球科学) » S-IT 地球内部科学・地球惑星テクトニクス

[S-IT19] 地球深部科学

2022年5月30日(月) 11:00 〜 13:00 オンラインポスターZoom会場 (22) (Ch.22)

コンビーナ:太田 健二(東京工業大学理学院地球惑星科学系)、コンビーナ:河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)、飯塚 毅(東京大学)、コンビーナ:土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、座長:太田 健二(東京工業大学理学院地球惑星科学系)、土屋 旬(愛媛大学地球深部ダイナミクス研究センター)、飯塚 毅(東京大学)、河合 研志(東京大学大学院理学系研究科地球惑星科学専攻)

11:00 〜 13:00

[SIT19-P13] Elasticity of Phase H under the Mantle Temperatures and Pressures: Implications for Discontinuities and Water Transport in the Mid-Mantle

*Zijun Song1Zhongqing Wu1 (1.University of Science and Technology of China)

キーワード:phase H, elasticity, water transport, discontinuities

Dense hydrous magnesium silicates (DHMSs) are considered to be the main carriers for transporting water to the Earth’s interior. Phase H (MgSiO4H2), as one of the deepest forms of DHMSs, contains 15.3 wt% water and plays an important role in transporting water into the mid-mantle. In this work, we investigated the thermodynamic properties and elastic properties of phase H at high P-T conditions using first-principles calculations.
The dehydration of phase H into bridgmanite, which may occur at the depth of ~1300-1700 km in cold slabs, will cause an increase of 1.0%, 2.7%, 15% at 1500 km on VP, Vs, and density, respectively. The impedance contrast for shear wave velocity by the dehydration of phase H is ~17%. Combining our results with seismic observations, the dehydration of the moderate amount of phase H could generate the seismic discontinuities at the depth of ~1300-1700 km detected in some subduction zones. Besides, the anisotropy of phase H is remarkable at the depths where phase H could exist stably and could be observed within slabs by seismology. Our results provide evidence for water transport in the mid-mantle.